LRD Watch DR1 · candidate
LRDW J175327.59+650641.1
Images






3.2″ across, north up, east left, resampled from the deepest mosaic covering the object in each band; ticks mark the catalogue position. Each band is stretched on its own noise; the composite shares one flux scale, so its colour is real. No coverage in F277W, F410M.
Spectral energy distribution
- NIRCam wide
- MIRI
- 2σ upper limit (S/N < 2)
At a glance
- Tier
- SILVER z < 3 BH* class
- Found by
- BH* channel
- Redshift
- 2.44 BH* fit
- Spectral shape
- no labelled spectrum
- F444W
- 22.15 AB S/N 217, 0.16″ aperture
- F277W − F444W
- not in the colour lane
- BH* share
- 0.81 cliff_degraaff25; Δχ² galaxy 41.2, dwarf 66.7
- Compactness
- growth ratio 2.174 stars 1.762
- Balmer break
- 4.72 ± 0.30 F150W/F115W, clean
- Image vetting
- half-stack pass; no flags raised
- Literature
- no published match within 1″
Vetting
- Image vettingpassed
- Half-stack testpass
- Artifact risknone
- Neighbournone
- Extendedno
- No vetting notes.
Redshifts
Each redshift keeps its own column. Photometric redshifts of little red dots are unreliable: against spectra, about a third of AGN-template redshifts (z_agn; 31 of 95 in the last purity run) and about half of galaxy-template redshifts at z > 3 were catastrophic outliers (methods Section 8).
| Column | What it is | z | Source |
|---|---|---|---|
z_spec | Spectroscopic, DJA grade 3 | — | — |
z_vet | Adopted by vetting | 2.4409 | bhstar:cliff_degraaff25 |
z_phot | Photometric (P(z) peak) | — | not fitted |
z_bhs | BH* channel fit | 2.441 | cliff_degraaff25 |
z_agn | Colour-lane fit | — | — |
Spectral checks
- V-shape (spectrum)
- no labelled spectrum
- Star (spectrum)
- no spectrum
- V-shape (photometry)
- not measurable βUV not measured, βopt not measured at z_agn
- Line in F410M
- none 2 line-free optical band(s)
- Line-ambiguous
- no
- Settling verdict
- not evaluated
Literature
Published objects within 1″ of this position. A match is a positional recovery, not an adopted classification.
- No published JWST little red dot or broad-line AGN within 1″.
Photometry
Circular aperture of radius 0.16″ at each band's native resolution, background from a 0.40–0.65″ annulus, programmes combined by inverse variance. For a point source multiply by the field's aperture correction (r = 0.16″ → 0.70″). Grey rows are below S/N 2.
| Band | Instrument | Pivot (µm) | f (nJy) | σ (nJy) | AB mag | S/N | Ap. corr. |
|---|---|---|---|---|---|---|---|
| F090W | NIRCam wide | 0.902 | 57.22 | 17.54 | 27.01 | 3.3 | 1.15 |
| F115W | NIRCam wide | 1.154 | 236.44 | 14.84 | 25.47 | 15.9 | 1.12 |
| F150W | NIRCam wide | 1.501 | 1115.95 | 13.45 | 23.78 | 83.0 | 1.11 |
| F200W | NIRCam wide | 1.989 | 2251.98 | 11.94 | 23.02 | 188.7 | 1.09 |
| F356W | NIRCam wide | 3.568 | 4593.36 | 16.29 | 22.25 | 282.0 | 1.23 |
| F444W | NIRCam wide | 4.404 | 5034.58 | 23.21 | 22.14 | 216.9 | 1.27–1.28 |
| F1000W | MIRI | 9.947 | 1249.87 | 55.44 | 23.66 | 22.6 | 2.45 |
Provenance
- Field
- NEXUS (
nexuscenter) - Programmes
05105, 09263behind every mosaic the field measured- Pipeline rows merged
- 1 all at one position
- Detection pass
- original
- Release build
33af9933d1cc2026-10-17T14:29:44Z
Image sources
| Band | Mosaic | Native pixel | Coverage |
|---|---|---|---|
| F090W | jw05105-o014_t001_nircam_clear-f090w_i2d.fits | 0.031″ | 1.00 |
| F115W | jw09263-o001_t001_nircam_clear-f115w_i2d.fits | 0.031″ | 1.00 |
| F150W | jw09263-o001_t001_nircam_clear-f150w_i2d.fits | 0.031″ | 1.00 |
| F200W | jw09263-o001_t001_nircam_clear-f200w_i2d.fits | 0.031″ | 1.00 |
| F356W | jw09263-o001_t001_nircam_clear-f356w_i2d.fits | 0.063″ | 1.00 |
| F444W | jw05105-o014_t001_nircam_clear-f444w_i2d.fits | 0.063″ | 0.54 |
Cite
Anderson, Jordan (2026). LRD Watch DR1: little red dot candidates from an independent search of public JWST imaging (Version DR1) [Data set]. Cerin Amroth Research. Zenodo. https://doi.org/10.5281/zenodo.23062632 Object LRDW J175327.59+650641.1.
CC BY 4.0. Please also acknowledge the JWST programmes that took the data. LRD Watch DR1 is a vetted candidate catalogue, not a complete census: it has no selection function and cannot on its own give number densities. About the release.